Heliacal Rising & Setting – Fixed Stars

Track when fixed stars emerge from and disappear into the Sun's light.

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Calculation Parameters
Location: Unknown (, ), Elevation: 0m
Visibility Model: Naked-eye photometric model
Atmosphere: 1013.25 mbar, 15°C, 40% humidity, κ=0.18
Observer: Naked eye, Snellen 1.5

Note: This models a clear dark sky with good eyesight.

Heliacal Events

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Methodology: Fixed star heliacal events calculated using Swiss Ephemeris apparent positions, Garstang atmospheric extinction, and Schaefer (1993) photometric visibility. Accounts for atmospheric conditions, observer acuity, and your exact location.

Accurate.
Simple.
Capable.

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A Couple
of Things

What is a fixed star heliacal rising?

A fixed star's heliacal rising occurs when it first becomes visible in the pre-dawn sky after being hidden by the Sun's light. This annual event was critical in ancient astronomy for marking seasons and was used in medieval astrology to assess the star's influence on mundane and natal charts.

What is a fixed star heliacal setting?

A fixed star's heliacal setting is its last visible appearance in the evening sky before it disappears into the Sun's glare. After its heliacal setting, the star enters a period of invisibility until it re-emerges at its next heliacal rising.

Which fixed stars are most important in astrology?

The most significant fixed stars include the four Royal Stars (Aldebaran, Regulus, Antares, Fomalhaut), as well as Sirius, Spica, Algol, Vega, Arcturus, and others. Each carries distinct significations based on centuries of astrological observation.

Why does location affect fixed star visibility?

Your geographic latitude determines which stars are visible and when they rise or set heliacally. Stars near the southern celestial pole (like Canopus) are only visible from southern latitudes, while stars near the northern pole may never set at high northern latitudes.

How often do fixed stars rise and set heliacally?

Each fixed star has one heliacal rising and one heliacal setting per year. The dates shift by about 1 day every 72 years due to precession of the equinoxes.

How accurate are these calculations?

Swiss Ephemeris's heliacal visibility algorithm accounts for atmospheric extinction, observer acuity, and your exact geographic coordinates to determine when each star becomes visible or disappears.